This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8559,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3559 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J181340-1913.1,2461139.8559,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J181340-1913.1 20260409.3559 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173654.71-165505.2,2461139.8559,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173654.71-165505.2 20260409.3559 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V4724 Sgr,2461139.8559,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V4724 Sgr 20260409.3559 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 17 50 08.78 -15 51 12.3 13.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4148032964493377280,2461139.8559,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4148032964493377280 20260409.3559 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4124809693983945728,2461139.8559,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4124809693983945728 20260409.3559 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4071231699307217792,2461139.8559,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4071231699307217792 20260409.3559 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.6419-21.8447,2461139.8559,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.6419-21.8447 20260409.3559 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4116570606690764800,2461139.8559,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4116570606690764800 20260409.3559 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J181834-2302.5,2461139.8559,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J181834-2302.5 20260409.3559 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181649.77-230307.8,2461139.8559,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181649.77-230307.8 20260409.3559 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181739.07-224634.9,2461139.8559,12.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181739.07-224634.9 20260409.3559 12.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8559,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3559 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181625.78-180710.1,2461139.8559,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181625.78-180710.1 20260409.3559 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4144006312337229184,2461139.8559,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4144006312337229184 20260409.3559 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1928 Oph,2461139.8559,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1928 Oph 20260409.3559 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8559,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3559 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4123470836719430912,2461139.8559,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4123470836719430912 20260409.3559 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175450.86-213712.7,2461139.8559,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175450.86-213712.7 20260409.3559 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172450.93-221755.9,2461139.8559,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172450.93-221755.9 20260409.3559 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1872 Oph,2461139.8559,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1872 Oph 20260409.3559 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2948 Oph,2461139.8559,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2948 Oph 20260409.3559 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175710.38-204753.1,2461139.8559,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175710.38-204753.1 20260409.3559 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173920.61-164106.1,2461139.8559,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173920.61-164106.1 20260409.3559 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J180258-2201.9,2461139.8559,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180258-2201.9 20260409.3559 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FK Sgr,2461139.8559,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FK Sgr 20260409.3559 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173608.39-211557.3,2461139.8559,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173608.39-211557.3 20260409.3559 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174837.87-180456.8,2461139.8559,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174837.87-180456.8 20260409.3559 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J174113-1639.7,2461139.8559,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J174113-1639.7 20260409.3559 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173749.35-205152.0,2461139.8559,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173749.35-205152.0 20260409.3559 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173314-2112.0,2461139.8559,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173314-2112.0 20260409.3559 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4090421235269879808,2461139.8559,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4090421235269879808 20260409.3559 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175026-1810.7,2461139.8559,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175026-1810.7 20260409.3559 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 17 25 42.03 -14 14 55.9 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SV Ser,2461139.8559,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SV Ser 20260409.3559 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173707.84-224845.2,2461139.8559,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173707.84-224845.2 20260409.3559 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4118682493692007424,2461139.8559,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4118682493692007424 20260409.3559 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174832.78-210623.0,2461139.8559,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174832.78-210623.0 20260409.3559 12.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J171339.08-192511.1,2461139.8559,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J171339.08-192511.1 20260409.3559 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172455.26-190321.6,2461139.8559,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172455.26-190321.6 20260409.3559 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J263.5542-16.4621,2461139.8559,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J263.5542-16.4621 20260409.3559 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 17 57 02.98 -15 52 42.4 12.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175702.88-155241.9,2461139.8559,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175702.88-155241.9 20260409.3559 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16621186,2461139.8559,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16621186 20260409.3559 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175920-2239.8,2461139.8559,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175920-2239.8 20260409.3559 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180311.66-200510.7,2461139.8559,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180311.66-200510.7 20260409.3559 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173249-2142.0,2461139.8559,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173249-2142.0 20260409.3559 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174404.17-191302.2,2461139.8559,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174404.17-191302.2 20260409.3559 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-ECL-068917,2461139.8559,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OGLE-BLG-ECL-068917 20260409.3559 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175338-2222.6,2461139.8559,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175338-2222.6 20260409.3559 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175158.04-225919.1,2461139.8559,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175158.04-225919.1 20260409.3559 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J180001-2249.2,2461139.8559,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180001-2249.2 20260409.3559 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175407-2303.5,2461139.8559,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175407-2303.5 20260409.3559 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2746 Oph,2461139.8559,10.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2746 Oph 20260409.3559 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4119192976274495104,2461139.8559,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4119192976274495104 20260409.3559 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180901.40-191852.1,2461139.8559,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180901.40-191852.1 20260409.3559 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J180613-2117.0,2461139.8559,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J180613-2117.0 20260409.3559 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174020.19-191802.7,2461139.8559,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174020.19-191802.7 20260409.3559 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175419-2226.0,2461139.8559,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175419-2226.0 20260409.3559 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8559,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.3559 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174327.53-212525.9,2461139.8559,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174327.53-212525.9 20260409.3559 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175734-1932.3,2461139.8559,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175734-1932.3 20260409.3559 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173502.10-215757.9,2461139.8559,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173502.10-215757.9 20260409.3559 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VV Sgr,2461139.8559,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VV Sgr 20260409.3559 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J174519-1741.9,2461139.8559,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J174519-1741.9 20260409.3559 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4120270463310928000,2461139.8559,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4120270463310928000 20260409.3559 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4069489316933491200,2461139.8559,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4069489316933491200 20260409.3559 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4090741845985461120,2461139.8559,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4090741845985461120 20260409.3559 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180748.83-162422.8,2461139.8559,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180748.83-162422.8 20260409.3559 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 21768,2461139.8559,10.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 21768 20260409.3559 10.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173845.58-223310.3,2461139.8559,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173845.58-223310.3 20260409.3559 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175820-2242.9,2461139.8559,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175820-2242.9 20260409.3559 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 18 12 27.60 -15 12 04.8 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146028554758488064,2461139.8559,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146028554758488064 20260409.3559 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175547.35-222613.7,2461139.8559,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175547.35-222613.7 20260409.3559 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4096393576230574336,2461139.8559,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4096393576230574336 20260409.3559 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172918.71-211921.8,2461139.8559,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172918.71-211921.8 20260409.3559 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J259.2154-20.2769,2461139.8559,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J259.2154-20.2769 20260409.3559 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.2702-22.2876,2461139.8559,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.2702-22.2876 20260409.3559 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 17 53 09.81 -15 19 33.1 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UX Ser,2461139.8559,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UX Ser 20260409.3559 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172824.00-185428.9,2461139.8559,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172824.00-185428.9 20260409.3559 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181419.71-212932.0,2461139.8559,12.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181419.71-212932.0 20260409.3559 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J273.5587-22.5595,2461139.8559,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J273.5587-22.5595 20260409.3559 11.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181757.46-220114.4,2461139.8559,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181757.46-220114.4 20260409.3559 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173050-1927.9,2461139.8559,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173050-1927.9 20260409.3559 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 16612284,2461139.8559,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 16612284 20260409.3559 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175006.14-203115.6,2461139.8559,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175006.14-203115.6 20260409.3559 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095593922006889344,2461139.8559,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095593922006889344 20260409.3559 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J262.4478-20.3795,2461139.8559,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J262.4478-20.3795 20260409.3559 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172822.89-174143.3,2461139.8559,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172822.89-174143.3 20260409.3559 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J260.4137-20.5400,2461139.8559,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J260.4137-20.5400 20260409.3559 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175458-2021.0,2461139.8559,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J175458-2021.0 20260409.3559 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173452-1958.6,2461139.8559,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173452-1958.6 20260409.3559 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2917 Oph,2461139.8559,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2917 Oph 20260409.3559 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J172743.69-220202.9,2461139.8559,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J172743.69-220202.9 20260409.3559 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2557 Oph,2461139.8559,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2557 Oph 20260409.3559 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175315.40-203801.6,2461139.8559,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J175315.40-203801.6 20260409.3559 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V3908 Sgr,2461139.8559,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V3908 Sgr 20260409.3559 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J174305-2257.4,2461139.8559,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J174305-2257.4 20260409.3559 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J173650.95-195338.0,2461139.8559,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J173650.95-195338.0 20260409.3559 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.3559* 18 01 11.73 -15 20 32.2 12.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4145459072117841024,2461139.8559,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4145459072117841024 20260409.3559 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174431.15-201143.7,2461139.8559,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J174431.15-201143.7 20260409.3559 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461139.85628569 09.04.2026 08:32:53.084 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.25
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15230
Objects passed selection criteria: 15213
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 13768.8
Average stars matched: 13361.5 (97.0422 %)
Memory usage VmPeak: 121892 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 03:34:59 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461139.85628569 09.04.2026 08:32:53.084 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 472
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 84 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 162839
Objects passed selection criteria: 162465
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 135261
Average stars matched: 129125 (95.4636 %)
Memory usage VmPeak: 1924376 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 03:39:35 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
SExtractor catalog cache: saved Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461139.85545819
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits'
wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:38.410 -18:00:45.25
Angular distance between the image centers 0.0802 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:36.098 -18:00:18.00
Angular distance between the image centers 0.0714 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:46:38.410 -18:00:45.25
Second-epoch second image center 17:46:36.098 -18:00:18.00
Angular distance between the image centers 0.01188 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.hy4hqCxAxH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.d22GyqrGmk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits &> /tmp/tmp.oaLPBJ5S0L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits &> /tmp/tmp.2KtzX1UxgU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 15752 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 258.0365 to 275.0296 deg, Dec -23.3066 to -12.5656 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 258.0365 to 275.0296 deg, Dec -23.3066 to -12.5656 deg
Loaded 14544 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9713 out of 10414 total matches.
Matched with Tycho-2 10414 out of 15752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854386
a=0.000000 b=1.000000 c=22.854386
From vast_summary.log: estimated ref. image limiting mag.: -8.25
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 34 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
2.3 pix Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
3.8 pix fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
3.8 pix fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Limiting magnitude estimates:
14.6 mag. Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.6 mag. Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
14.0 mag. fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
14.0 mag. fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.hy4hqCxAxH (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1456, passed=15752
Got 15752 stars (including 14271 good ones) from the SExtractor catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 15752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 870 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 14813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 14813 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 14814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.d22GyqrGmk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1474, passed=15602
Got 15602 stars (including 14101 good ones) from the SExtractor catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 15602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 14412 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 14410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 14411 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 916 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.oaLPBJ5S0L (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Checking if the catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS catalog name: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=688, passed=11985
Got 11985 stars (including 11290 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat
util/solve_plate_with_UCAC5 got 11985 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 11727 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 11728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 11728 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits -region wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2KtzX1UxgU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Checking if the catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS catalog name: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=691, passed=12072
Got 12072 stars (including 11371 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat
util/solve_plate_with_UCAC5 got 12072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 11797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 332 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 11792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 11792 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 914 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits -region wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits'
Preparing the HTML report for the field Sgr-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21425.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21428.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21485.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21496.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21514.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21433.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 21052_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21052_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:49.56 -17:31:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21114_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21114_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:45.76 -13:46:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21204_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 21204_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 21205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:08:28.74 -23:14:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21252_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21252_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:45.03 -13:47:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21306_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 21306_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 21327_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21327_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 21332_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21332_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:50:37.96 -17:56:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 0.825 4120499161734168448 267.65836220666 -17.94124472781 9.5710 8.0722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21364_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21364_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:26.70 -15:24:56.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 21393_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21393_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:00.78 -16:46:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.42, MAG_FAINT_SEARCH_LIMIT=12.40)GAIADR2_OUTPUT=# 1.563 4124036020120063616 265.75354501518 -16.77746873885 11.0008 10.0947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21408_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21408_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:10.68 -14:56:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21420_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21420_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:47:19.03 -17:30:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.612 4120750198363933056 266.82998308437 -17.51291948263 9.8722 8.4305 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21425_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21425_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:31:15.36 -21:35:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.992 4117864152129970432 262.81393748589 -21.59621383330 10.1883 8.7303 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21428_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21428_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:30.07 -20:41:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 0.978 4118182392053069568 265.37555031269 -20.68967880366 10.3023 8.9344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.978#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21433_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 21433_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 21437_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21437_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:18:55.70 -17:55:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21446_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21446_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:02:00.78 -15:16:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21471_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21471_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:27.19 -20:56:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21473_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21473_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:29.25 -14:49:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.043 4137048259154631168 261.87216408982 -14.82632601775 10.7590 9.4717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21474_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21474_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:00:34.73 -22:59:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 3.342 4069438430158980864 270.14559350638 -22.99177726607 10.8055 9.3452 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.342#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21477_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21477_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:36.33 -16:55:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 0.819 4144810806934944000 267.40153421242 -16.93308578286 11.3220 10.8837 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21480_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21480_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:52.39 -16:33:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 1.528 4124068009041373568 266.21863575712 -16.55890615272 11.3675 10.9340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21481_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21481_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:57.06 -20:40:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.998 4091336990952077824 274.48804636478 -20.66694775180 10.8863 9.6485 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21485_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21485_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:12.69 -18:59:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.70, MAG_FAINT_SEARCH_LIMIT=12.68)GAIADR2_OUTPUT=# 1.059 4122197671012278272 260.80316926013 -18.98465125472 11.2209 10.3051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21490_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21490_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:00.13 -17:45:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.121 4122757322456023808 262.25086823320 -17.75382153791 11.2965 10.3817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21496_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21496_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:31.13 -17:03:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 0.886 4123932837844294272 265.37996529144 -17.05478970130 11.1887 10.2255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21499_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21499_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:59.09 -17:43:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21501_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21501_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:28.95 -19:16:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 4.881 4121747695897972224 262.36991350908 -19.27557224393 11.4129 10.5539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21511_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21511_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:29.39 -16:25:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.721 4124108755326844032 265.37276376064 -16.43137782744 11.6457 11.2928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21514_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21514_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:59.87 -23:11:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 0.898 4066394604106345472 273.74932555950 -23.18500475474 11.1079 10.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21516_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21516_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:01.59 -15:28:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 1.948 4124990288769082624 265.25709967786 -15.48190020187 11.2647 10.2761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:13:38.12 -21:15:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21518_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21518_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:18:52.22 -22:00:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.762 4114939313728480768 259.71778635012 -22.00748544587 11.3310 10.4676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.762#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 06388_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 06388_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 14s
Prepared the HTML report for the field Sgr-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:11:57.48 -18:52:13.9
17:58:42.50 -19:19:43.1
18:13:39.51 -19:13:06.9
17:36:54.51 -16:54:59.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
SExtractor catalog cache: saved Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits exists and is non-empty
wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:38.410 -18:00:45.25
Angular distance between the image centers 0.0802 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:36.098 -18:00:18.00
Angular distance between the image centers 0.0714 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:46:38.410 -18:00:45.25
Second-epoch second image center 17:46:36.098 -18:00:18.00
Angular distance between the image centers 0.01188 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.f2V4xnjCuk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.SfMEgx3kmz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits &> /tmp/tmp.kN7NUjAU1U
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits &> /tmp/tmp.toy8AFCjrg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 179796 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 258.0045 to 275.0499 deg, Dec -23.3098 to -12.5486 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 258.0045 to 275.0499 deg, Dec -23.3098 to -12.5486 deg
Loaded 14601 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 9967 out of 12785 total matches.
Matched with Tycho-2 12785 out of 179796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.629045
a=0.000000 b=1.000000 c=22.629045
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.70
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.70
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 410 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
1.9 pix Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
3.2 pix fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
3.1 pix fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Limiting magnitude estimates:
14.7 mag. Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.7 mag. Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
14.0 mag. fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
14.0 mag. fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.f2V4xnjCuk (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=17851, passed=179759
Got 179759 stars (including 161611 good ones) from the SExtractor catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 179759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 877 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 169384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 169386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 169384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Excluding outliers - 918 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.SfMEgx3kmz (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=17987, passed=181044
Got 181044 stars (including 162789 good ones) from the SExtractor catalog wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 181044 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 881 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 919 matched stars entering correct_measured_positions(), 168120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 168121 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.45"
Accuracy estimation diagnostic: 918 matched stars entering correct_measured_positions(), 168120 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 918 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.kN7NUjAU1U (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Checking if the catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
WCS catalog name: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=7072, passed=91215
Got 91215 stars (including 84044 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat
util/solve_plate_with_UCAC5 got 91215 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 916 matched stars entering correct_measured_positions(), 89770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 89768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 89768 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits -region wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.toy8AFCjrg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Checking if the catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat corresponding to the image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
WCS catalog name: wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=7145, passed=92270
Got 92270 stars (including 85027 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat
util/solve_plate_with_UCAC5 got 92270 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 917 matched stars entering correct_measured_positions(), 90756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 331 to 391 (Dec -23.6 to -12.1)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 90756 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 915 matched stars entering correct_measured_positions(), 90753 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 915 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits -region wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_Sgr-01-Q1b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_Sgr-01-Q1b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-31-41_20.00sec_-4.90C_LIGHTs_0222.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sgr-01-Q1b1x1_033342_TTUQ1b1x1_3279_VIqMi3jm/wcs_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223.fits
Preparing the HTML report for the field Sgr-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out02510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out04506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out17938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191112.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191310.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out210980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out210994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out210995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211013.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211020.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211060.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211110.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211126.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211520.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211641.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211963.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out211991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212168.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212434.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212783.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212975.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out212977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213289.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213293.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213359.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213417.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213466.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213519.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213528.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213550.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213568.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213634.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out213731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out68111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out83193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out93019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out211005.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out212285.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out212526.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out05958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06196.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out08677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09448.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135838.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out149124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out191795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out211517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out213492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out26893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41601.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43788.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out47673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51273.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97529.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 65s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 51s
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Considering the candidate 210980_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 210980_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:47:36.02 -19:36:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.561 4119847220051177088 266.89935004592 -19.61321857780 13.1576 12.0364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 210992_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 210992_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 210994_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 210994_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:30.04 -16:15:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.794 4136135492696005504 259.37634005959 -16.25331740149 13.9143 13.0114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 210995_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 210995_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:29.81 -16:15:26.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 211004_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211004_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:26.16 -17:44:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 4.781 4122898094291258112 260.86039425929 -17.74976984080 12.7911 11.4171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211005_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211005_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:10.04 -15:45:28.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 211007_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211007_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:10.77 -20:28:26.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 211012_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211012_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:10.34 -16:36:53.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 211013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:19.67 -20:09:05.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 211016_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211016_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:59:46.28 -15:04:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211017_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211017_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:56.41 -18:55:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 0.652 4123123627264479104 263.98493097592 -18.92979660481 13.1491 12.2899 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 211020_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211020_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:32.91 -16:20:44.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
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Considering the candidate 211025_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211025_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:43.31 -22:58:40.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 211028_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211028_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211029_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211029_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211030_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211030_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:17.35 -14:58:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.188 4136479090075605248 259.07256954885 -14.98091905466 13.0124 11.8773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211036_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211036_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:28.62 -13:03:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211038_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211038_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:10.97 -17:22:14.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 211041_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211041_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:57.55 -20:51:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211043_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211043_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211045_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211045_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:07:14.04 -21:03:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.054 4094076832160833152 271.80893181205 -21.06644081547 12.5151 11.5712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211048_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211048_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:28.25 -16:24:43.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 211049_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211049_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:38.26 -12:35:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.648 4141544230897820160 259.16021758724 -12.58406167359 13.4131 12.6836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211053_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211053_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:16.62 -13:37:39.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
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Considering the candidate 211054_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211054_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:21:38.05 -14:26:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211057_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211057_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:48:46.63 -16:11:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)
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Considering the candidate 211060_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211060_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:01:06.83 -21:00:05.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 211061_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211061_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:37.45 -15:23:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.770 4148225752608384640 266.15702327697 -15.38722622581 12.0739 10.6517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211062_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211062_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:46.41 -13:03:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.214 4141313058579401856 259.44351630800 -13.06410893811 13.0027 11.9887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.214#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211065_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211065_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:16:41.94 -14:50:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211068_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211068_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:32.87 -12:46:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.957 4141654383922074624 260.13708213060 -12.77897441997 13.0274 12.1388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.957#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211069_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211069_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211070_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211070_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:03:12.49 -20:18:37.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 211073_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211073_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:52:17.21 -18:04:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211078_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211078_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:04:40.99 -15:13:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 1.856 4146763715713355136 271.17044892147 -15.22392344341 11.8515 10.3197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211080_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211080_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:02.64 -19:18:41.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 211081_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211081_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:14.46 -14:02:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211083_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211083_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:01.89 -20:23:33.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)
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Considering the candidate 211087_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211087_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:59:41.02 -21:00:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 211088_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211088_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:12:43.68 -15:52:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.400 4145778205359740416 273.18298916476 -15.86885027349 13.0365 12.4756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211089_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211089_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:46.76 -13:31:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211090_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211090_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:52:20.87 -21:37:38.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 211091_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211091_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 211094_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211094_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:00:16.42 -16:16:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211096_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211096_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:05.62 -18:40:06.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 211098_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211098_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:09.08 -13:20:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211099_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211099_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:15.85 -20:16:03.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 211100_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211100_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:15:22.48 -22:02:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211101_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211101_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:08.73 -15:10:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.499 4145843557588549760 273.53716891987 -15.18440476280 12.8050 11.8771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.499#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211105_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211105_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:57:00.82 -20:28:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211106_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211106_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:27.23 -18:49:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 4.199 4094815188580353024 274.36452492670 -18.83052856656 12.3235 11.7577 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.199#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211108_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211108_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:24.73 -17:59:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.176 4096409313038370944 274.60253541295 -17.99378859351 12.7065 12.2397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.176#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211110_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211110_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:12:57.45 -21:47:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.878 4115420070845863552 258.23980752052 -21.78941616978 12.7604 11.8471 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211113_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211113_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:10:34.22 -15:42:12.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)
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Considering the candidate 211114_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211114_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 211115_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211115_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:15:16.06 -22:25:56.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)
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Considering the candidate 211116_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211116_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:20.51 -22:06:43.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)
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Considering the candidate 211118_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211118_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 211120_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211120_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:16:19.50 -21:37:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 3.009 4090841416116628608 274.08159362889 -21.63249448133 11.6914 10.6048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211123_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211123_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:06.53 -20:19:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.92, MAG_FAINT_SEARCH_LIMIT=12.90)GAIADR2_OUTPUT=# 2.740 4094362395945528960 274.27648660759 -20.31801489404 11.9963 11.1544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.740#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:07.76 -13:23:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211125_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211125_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:03:04.20 -22:44:34.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 211126_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211126_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:18.40 -21:53:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.329 4090633922025084544 274.57667100643 -21.89621416275 11.3926 10.5860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211127_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211127_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:27.20 -18:24:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211128_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211128_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:42.10 -16:31:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.979 4097609601694464896 274.67569941078 -16.52236570996 11.1625 10.5078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.979#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211130_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211130_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:37.49 -20:02:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 1.500 4116209077845017984 258.90659306330 -20.05001305938 11.2468 10.7074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211131_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211131_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:24.14 -23:10:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.79, MAG_FAINT_SEARCH_LIMIT=11.77)GAIADR2_OUTPUT=# 4.004 4066436488628605696 273.60000121945 -23.17816376865 10.6413 10.1271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211132_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211132_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:49.58 -17:31:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211163_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211163_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:01.06 -15:28:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211202_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211202_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:42.17 -13:46:51.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211284_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211284_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:58:42.51 -19:19:43.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 211302_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211302_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:08:28.77 -23:14:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211317_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211317_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:06:19.54 -16:41:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.820 4144307372386827392 271.58164392360 -16.68821053425 9.5088 8.0874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211376_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211376_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:28.11 -22:56:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.90, MAG_FAINT_SEARCH_LIMIT=11.88)GAIADR2_OUTPUT=# 0.782 4090430130047668992 274.61696313876 -22.93436966229 10.6776 10.4528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211405_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211405_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:02:30.62 -23:00:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 211517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 211520_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211520_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:29.04 -22:52:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.32, MAG_FAINT_SEARCH_LIMIT=12.30)GAIADR2_OUTPUT=# 1.542 4090432092859708928 274.62146090911 -22.87819561616 10.8583 10.0302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:30.63 -16:24:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211579_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211579_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:36.94 -22:56:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 0.572 4090410205747348736 274.40383790508 -22.93378010105 11.2665 10.7493 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211614_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211614_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:59.51 -17:21:56.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211615_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211615_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:59.89 -23:11:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.060 4066394604106345472 273.74932555950 -23.18500475474 11.1079 10.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211641_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211641_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:29.58 -23:06:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 4.715 4089650889913857280 274.62452453883 -23.10997268239 10.9264 9.7388 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211657_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211657_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:16:39.94 -23:10:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 1.148 4090399416786028672 274.16646945503 -23.16814859938 11.2960 10.9729 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211666_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211666_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:35.71 -16:44:00.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211676_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211676_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:52.10 -14:24:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211694_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211694_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:04.91 -15:47:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211726_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211726_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:25:59.40 -14:03:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211734_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211734_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:55.79 -14:48:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211790_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211790_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:13.54 -16:47:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211856_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211856_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:24.60 -22:53:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.051 4090411270899379584 274.35300278103 -22.89802625873 11.4224 10.7104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211860_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211860_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:35.89 -22:34:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 5.065 4090456660129540864 274.65099272667 -22.58320679090 11.1504 9.8910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:35.43 -21:53:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 3.566 4090634536130778368 274.64780315318 -21.88675430762 11.7757 11.1454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211900_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211900_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:19:03.19 -18:32:47.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211909_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211909_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:38.60 -13:45:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 2.135 4146612425449995776 274.66027303198 -13.76562462295 12.3193 11.6006 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211960_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211960_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:00.60 -18:23:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211963_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211963_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:08:24.03 -23:14:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 5.788 4066575812965465600 272.09858708294 -23.24085033346 11.7685 11.2154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 211970_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211970_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:34:56.89 -15:44:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 211991_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211991_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:26.32 -23:07:50.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)
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Considering the candidate 211993_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 211993_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:09.32 -20:30:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212018_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 212018_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 212047_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212047_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:14.51 -14:20:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212066_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212066_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:01.93 -13:23:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212108_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212108_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:13:01.71 -17:25:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212120_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212120_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:31.53 -22:21:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 5.500 4090558326231099392 274.63270517081 -22.35765578870 11.5906 10.4700 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212168_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212168_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:18.75 -22:50:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.731 4090431641876151936 274.57789209533 -22.84643013546 11.6896 11.1931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212201_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212201_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:58.04 -15:01:19.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:32.59 -17:53:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212214_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212214_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:55:50.81 -23:13:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212224_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212224_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:24.36 -22:19:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.390 4090558669828482048 274.60165968356 -22.32673063262 11.7409 10.9444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212250_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212250_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:11.57 -22:46:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 2.426 4090425079166118272 274.29880076371 -22.76828352024 11.6839 10.8986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.426#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212255_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212255_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:56:25.71 -16:13:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212279_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212279_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:37.59 -16:00:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212285_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212285_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:51.56 -21:49:42.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)
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Considering the candidate 212302_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212302_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:01.23 -23:05:16.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)
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Considering the candidate 212304_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212304_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:07.34 -23:05:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)GAIADR2_OUTPUT=# 2.051 4089654424600049280 274.53119187242 -23.09166180897 11.8537 11.0440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212328_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212328_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:25:14.56 -18:35:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212350_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212350_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:59:26.00 -15:09:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.337 4145502919491958144 269.85768580369 -15.15379665701 12.6364 11.8940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212357_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212357_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:32.87 -20:22:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212372_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212372_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:39.62 -19:31:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212403_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212403_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:03.63 -22:57:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 2.505 4090407177742441088 274.51467701040 -22.96053265070 11.8880 11.4768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.505#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212406_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212406_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:38.02 -17:12:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 0.771 4134848853626519936 258.90835526146 -17.20551611567 12.4549 11.5113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212408_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212408_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:06.03 -22:32:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 3.447 4090460882013476736 274.52465654581 -22.54585415143 12.0970 11.8332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212434_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212434_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:53.76 -16:26:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 4.100 4124108141219840384 265.47478101126 -16.44410798464 11.8077 10.1952 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212451_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212451_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:39.07 -14:42:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212473_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212473_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:01:12.78 -15:19:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.839 4145459110823234816 270.30372669984 -15.33181570902 12.6305 12.0736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212495_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212495_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:13:44.95 -18:21:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212511_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212511_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:11:13.58 -23:13:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212526_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212526_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:15:50.00 -23:10:18.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)
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Considering the candidate 212548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 212548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 212562_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212562_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:20.09 -14:59:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212564_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212564_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:02:54.08 -14:31:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212567_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212567_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:33:57.27 -13:28:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212603_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212603_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:05.55 -23:03:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 3.800 4090401955062211712 274.27408084185 -23.05191677697 12.1697 11.2978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212608_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212608_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:54:55.90 -15:21:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212645_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212645_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:05.98 -15:55:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212651_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 212651_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 212657_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212657_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:55.10 -18:19:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.846 4096382065762816640 274.47994926736 -18.32604399650 12.0532 10.4395 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212660_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212660_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:12:25.82 -15:25:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 4.556 4145997287393842816 273.10848211031 -15.42031120134 11.9204 10.4926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212681_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212681_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:15:02.32 -15:23:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212699_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212699_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:18:24.61 -12:50:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212705_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212705_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:40:29.71 -20:01:26.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
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Considering the candidate 212712_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212712_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:51.99 -15:50:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212729_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212729_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:21:38.35 -14:37:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 5.038 4137898933242348544 260.40917405393 -14.62676535999 13.1508 12.2673 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212762_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212762_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:30:14.62 -18:38:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212768_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212768_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:26:49.32 -14:16:03.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212783_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212783_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:04:53.49 -16:01:16.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 212785_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212785_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:56.59 -19:10:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212849_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212849_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:34:10.34 -20:13:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:28.62 -13:39:10.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212873_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212873_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:13:37.76 -19:56:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212884_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212884_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:40:16.27 -15:05:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212891_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212891_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:33:16.78 -16:36:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212892_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212892_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:13.30 -16:45:28.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212930_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212930_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:34:15.61 -19:06:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212946_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212946_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:54:34.02 -19:44:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212966_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212966_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:45.10 -17:43:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212975_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212975_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:52.24 -18:34:24.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 212977_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212977_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:51:06.92 -13:09:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.277 4149731400678554112 267.77907058191 -13.16054727356 13.4020 12.3591 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 212989_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 212989_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:34.33 -18:07:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213006_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213006_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:40.22 -22:36:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.250 4114742638576072192 260.91723019879 -22.60122772411 12.3087 10.7946 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:38.70 -13:36:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213032_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213032_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:45.03 -21:19:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.205 4090911544346695040 273.68908986082 -21.33070063817 12.1093 10.5770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 213067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 213076_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213076_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:53:16.57 -18:06:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213080_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213080_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:40.61 -15:16:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.290 4148979708344908160 266.16921500860 -15.27189192124 12.1971 10.6450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.290#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213082_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213082_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:26:31.87 -15:08:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213083_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213083_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:40:50.54 -16:21:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.668 4124123633093892480 265.21164518667 -16.35047935398 12.3668 10.4127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213086_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213086_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:19:12.21 -16:39:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213104_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213104_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:03:55.89 -15:23:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.802 4145258724854873856 270.98408876499 -15.39066517845 13.3164 11.1781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213109_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213109_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:33.92 -22:13:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213115_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213115_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:31.29 -22:22:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213118_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213118_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:26.96 -18:14:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:08:10.99 -14:34:29.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213128_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213128_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:51:38.45 -20:50:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.223 4118715822590570240 267.91045059607 -20.84508829673 12.1573 10.5229 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.223#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213139_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 213139_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 213149_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213149_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:04:28.52 -18:57:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 1.928 4095394669879067904 271.11916019158 -18.96097940982 12.2745 10.2990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213166_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 213166_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 213191_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213191_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:36:04.09 -19:43:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213198_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213198_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:01:15.38 -16:13:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 1.685 4145064076944721792 270.31456525082 -16.21737337347 13.8573 11.9632 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213205_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:52:06.87 -21:48:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 4.352 4070525086941221504 268.02966936194 -21.81344443466 11.3922 9.7192 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213206_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213206_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:28.68 -16:57:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213207_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213207_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:40:28.82 -13:34:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.432 4161481091160807296 265.11972273458 -13.57665230238 14.0299 13.1137 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213222_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213222_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:09.42 -21:18:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213233_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213233_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:14.10 -19:12:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213246_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213246_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:56.66 -22:16:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213249_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213249_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:30:17.03 -14:02:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213250_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213250_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:01.62 -19:13:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.429 4121616098129329408 263.75741197422 -19.22589261788 13.8316 11.8994 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.429#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213252_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213252_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:39.43 -23:02:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213257_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213257_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:00:33.26 -21:10:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213287_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213287_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:43.48 -20:58:53.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213289_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213289_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:55.60 -21:55:25.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 213292_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213292_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:39.24 -15:24:51.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 213293_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213293_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:04:16.40 -17:20:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.714 4143978854585965568 271.06837352179 -17.34505541679 11.8298 10.3312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213307_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213307_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:18.74 -23:04:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.856 4068825551199204736 266.07858236071 -23.06871019535 13.1767 11.7627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:59:02.15 -16:36:05.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213319_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213319_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:45:34.93 -15:03:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 0.910 4148989088554288000 266.39552801336 -15.05894701434 12.0047 10.4507 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213345_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213345_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:05.64 -13:29:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.898 4149485007002513280 266.02399674577 -13.48512180663 14.0660 12.1586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213353_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213353_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:03.00 -18:32:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 5.167 4122468288310994560 260.01205830812 -18.53726169204 13.0125 11.7187 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213359_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213359_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:50:56.46 -22:15:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.555 4070434759591624064 267.73510067612 -22.26006835478 14.4331 12.4842 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213377_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213377_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:10.91 -18:35:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213382_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213382_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:21.55 -17:06:27.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 213387_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213387_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:50:18.42 -15:39:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213390_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213390_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:56:22.68 -19:10:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.924 4119373674140029056 269.09531773954 -19.17747131263 12.7708 11.3499 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213391_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213391_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:25:45.59 -15:48:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.536 4136882301614888064 261.44000475069 -15.80455246463 12.7068 10.7369 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213405_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213405_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:03.83 -13:35:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213417_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213417_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:33:13.57 -18:50:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.198 4121834518599887488 263.30713420345 -18.84721380496 12.8992 11.2773 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.198#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213422_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213422_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:25:31.05 -18:00:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.580 4122922622808905344 261.37994221103 -18.01708296623 12.7353 11.3504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213424_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213424_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:03:07.45 -15:19:57.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 213443_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213443_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:48:09.86 -20:37:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.796 4118875737206838912 267.04122508453 -20.62550876740 14.3035 12.4569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213444_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213444_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:03:02.24 -21:05:29.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213447_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213447_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:15.39 -13:14:09.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213450_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213450_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:11.94 -19:23:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.015 4119906696763078144 266.05034092050 -19.38966086614 11.9268 10.3313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213457_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213457_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:11:09.22 -18:55:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 3.820 4095495133443044736 272.78951664974 -18.92151311434 11.8240 10.2827 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213458_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213458_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:15.97 -16:19:30.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213466_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213466_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:22:53.20 -20:18:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.292 4121206701820359808 260.72189497571 -20.30334953952 14.2158 12.4054 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213484_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213484_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:59.50 -22:30:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.586 4116777417954393344 264.74804735547 -22.51491461089 12.7572 11.3134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213492_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 213492_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 213494_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213494_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:54:52.61 -14:03:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213495_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213495_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:30:50.24 -22:44:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.320 4117499526570407168 262.70867551165 -22.73691660502 12.2475 10.6511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213499_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213499_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:28:25.25 -21:02:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 0.420 4120958620150417792 262.10530434776 -21.04399138061 13.0012 11.3979 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213506_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213506_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:14.09 -15:21:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.421 4125172124841429632 264.55909920834 -15.36379970457 13.0733 11.8718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213516_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213516_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:30.53 -21:51:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.786 4070512275101498112 267.37861124251 -21.85467671619 12.2050 10.4253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213519_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213519_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:21.55 -15:18:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.220 4148968541429837184 265.84021755625 -15.30673756530 12.9663 11.6152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213523_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213523_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:33.99 -19:52:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213528_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213528_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:51:06.33 -18:38:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.407 4120377768780951936 267.77657003067 -18.64633698191 12.1526 10.6226 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213534_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213534_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:11.35 -14:02:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213541_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213541_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:32.35 -15:28:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.534 4148247193081975296 267.38541884134 -15.48102727209 12.1795 10.7027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213547_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213547_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:26:33.66 -20:28:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.498 4121229138725014784 261.64063021755 -20.47871512501 13.6742 12.1313 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213550_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213550_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:14.31 -13:26:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.263 4149494730809193088 265.55969423650 -13.44459721420 12.6109 11.1923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213558_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213558_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:05.77 -20:34:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.990 4118220114642935040 264.77471377127 -20.57515302022 12.4027 10.8208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213560_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213560_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:33:47.95 -16:15:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.194 4124645351356746112 263.44997306983 -16.26383768675 12.2251 10.6465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213561_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213561_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:41:14.68 -14:33:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213568_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213568_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:35.20 -17:04:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.303 4123746367559887360 265.64761361916 -17.08020573290 11.7891 10.1261 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213578_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213578_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:55:08.20 -23:07:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 2.180 4070137165490190080 268.78401867661 -23.12009017306 12.5560 11.0050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213580_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213580_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:27.06 -21:41:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.714 4117299411116117632 265.61351857147 -21.69048106999 14.4716 12.8470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.714#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213587_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213587_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:50.62 -18:40:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.550 4123191938822381696 264.96190771065 -18.67037603313 13.2158 11.9610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213592_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213592_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:24.35 -16:24:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.673 4124592093769417344 262.35160605028 -16.41179490037 12.2115 10.6780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213621_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213621_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:34:14.60 -19:17:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.123 4121609226180578432 263.56173178543 -19.28359892012 12.7691 11.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213623_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213623_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:40:56.80 -19:56:44.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213629_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213629_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:58:13.48 -20:02:53.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 213631_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213631_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:00:02.81 -14:48:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.244 4145536969995649664 270.01250660412 -14.81215941950 12.7435 11.2829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213634_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213634_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:00.57 -20:29:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.261 4118411429666926080 264.50301732023 -20.49668064338 13.2644 11.8914 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213666_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213666_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:29.80 -16:01:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 1.822 4125028191901495040 263.87459249077 -16.02832559782 12.7760 11.3748 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213678_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213678_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:28.99 -14:31:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.996 4149313100886057984 264.62135308028 -14.51755648450 12.3494 10.7820 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213723_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213723_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:36:42.30 -17:16:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 1.101 4123595906264894080 264.17654618972 -17.27733847544 13.3243 11.7774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213728_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213728_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:30:47.99 -18:27:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.738 4121908529480102400 262.70016323051 -18.45448697079 12.8358 11.3435 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 213731_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 213731_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:25:49.50 -16:21:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 2.293 4136638102636668544 261.45649743031 -16.35410333220 12.7343 11.4158 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.293#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 83010_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 83010_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 194329_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 194329_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:04.13 -22:29:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.767 4116997530830683136 266.51766233965 -22.48372719294 11.8018 10.2711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 86018_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 86018_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:16.82 -17:55:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.671 4123478361586918272 264.57066587191 -17.92752112721 10.6185 9.2465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 27969_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 27969_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:36.43 -21:02:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22418_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 22418_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 11261_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 11261_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 63043_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 63043_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 104635_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 104635_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:24:28.99 -16:58:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55097_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 55097_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 34518_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 34518_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 33957_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 33957_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:20:58.95 -20:38:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 113067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 113067_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 48377_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 48377_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:33.57 -19:38:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132539_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 132539_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:02:04.73 -15:03:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 206599_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 206599_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:28:22.91 -15:40:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60437_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 60437_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:38:29.56 -19:05:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16586_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 16586_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 125524_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 125524_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 26748_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 26748_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 82886_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 82886_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191112_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191112_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:11:27.07 -22:32:28.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 113772_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 113772_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191475_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191475_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:13.39 -21:59:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.98, MAG_FAINT_SEARCH_LIMIT=11.96)GAIADR2_OUTPUT=# 1.227 4090629214737690112 274.30542966307 -21.98527391533 10.7922 10.5216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 32855_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 32855_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 27869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 27869_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191795_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 191795_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 81673_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 81673_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 130409_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 130409_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 25679_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 25679_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:19:58.06 -21:11:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44480_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 44480_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:21:49.38 -19:58:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199813_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 199813_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:56:17.20 -16:53:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05958_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 05958_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 194147_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 194147_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:36:00.23 -21:04:59.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 194109_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 194109_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:34:16.75 -22:21:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.30, MAG_FAINT_SEARCH_LIMIT=13.28)GAIADR2_OUTPUT=# 5.221 4117577724971719040 263.56955144802 -22.35390019393 12.2935 11.5675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 35010_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 35010_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 29870_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 29870_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 51273_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 51273_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 148752_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 148752_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:49:43.72 -15:52:01.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
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Considering the candidate 59807_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 59807_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 44393_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 44393_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:35:05.82 -20:06:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117094_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 117094_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 15323_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 15323_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:24:34.32 -21:59:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 149124_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 209487_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 209487_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:30:43.96 -18:54:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199911_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 199911_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:19:42.24 -14:55:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 04506_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 04506_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:06.10 -22:56:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.141 4116879814358009728 265.77666517193 -22.94842295784 11.6899 10.1572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111335_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 111335_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:45:29.50 -16:46:38.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)
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Considering the candidate 68111_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 68111_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:24.40 -18:39:27.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
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Considering the candidate 49274_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 49274_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 08283_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 08283_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 192274_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 192274_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:52:55.97 -22:53:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.443 4070200249968817792 268.23308602264 -22.89380808876 11.6557 9.9421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.443#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 13573_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 13573_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:20.18 -22:09:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65019_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 65019_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:30.18 -18:40:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 111310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:48:11.38 -16:47:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45429_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 45429_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 09637_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 09637_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:39:17.41 -22:32:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20322_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 20322_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 90291_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 90291_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:29:56.28 -17:40:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58754_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 58754_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191818_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191818_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:15.06 -22:02:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.835 4090614195165671936 274.56272925514 -22.04037057548 11.9228 11.3776 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 22259_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 22259_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:15:23.30 -21:26:15.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05758_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 05758_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 12308_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 12308_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 04300_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 04300_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 170707_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 170707_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:57:27.25 -14:22:37.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 93823_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 93823_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:19.01 -17:23:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06196_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 06196_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191538_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191538_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:32.52 -22:07:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.40, MAG_FAINT_SEARCH_LIMIT=12.38)GAIADR2_OUTPUT=# 0.923 4090623545380203520 274.38553263162 -22.12917119330 11.1733 10.9293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 03367_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 03367_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191465_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191465_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:26.45 -22:09:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.764 4090609247363353600 274.61071810062 -22.16357612813 11.2870 10.9860 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 97529_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 97529_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 43425_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 43425_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191349_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191349_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:17.53 -22:47:57.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)
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Considering the candidate 191310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191310_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:15:49.69 -22:08:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 5.098 4090715285901766144 273.95849008979 -22.13926890958 12.1552 11.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 56756_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 56756_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 99402_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 99402_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:33:36.91 -17:17:26.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26893_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 26893_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 56970_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 56970_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 191133_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191133_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:03.93 -15:26:01.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 191079_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191079_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:01.45 -18:32:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.067 4120217995993180672 265.50495530479 -18.54598022334 11.5120 10.0681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191076_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 191076_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:11.13 -21:28:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190972_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 190972_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:24.05 -13:07:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.043 4141311031354855680 259.35105469382 -13.11810419628 13.3561 12.2633 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.043#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 158517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 158517_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:11.43 -13:24:11.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 02510_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 02510_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:52:32.65 -23:08:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.438 4068647743953625856 268.13669691579 -23.13794833060 11.6046 9.9254 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 09055_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 09055_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:57.33 -22:36:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 21013_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:28:52.97 -21:37:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164079_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 164079_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:51:56.10 -13:52:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49619_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 49619_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:19:07.83 -19:36:03.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 11548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 160192_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 160192_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:32:08.66 -13:31:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190583_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 190583_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:31:56.06 -19:19:44.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104017_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 104017_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 25107_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 25107_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 53704_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 53704_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 178698_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 178698_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:44:10.69 -14:56:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17049_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 17049_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 04424_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 04424_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:17:24.78 -22:50:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177186_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 177186_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:14:02.67 -14:49:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56976_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 56976_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 87271_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 87271_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:02.54 -17:40:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51891_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 51891_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:18:51.32 -19:32:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 3.215 4094556219230848640 274.71467556590 -19.54235358476 12.1698 11.5986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91553_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 91553_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 136842_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 136842_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:02:00.79 -15:16:31.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13902_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 13902_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:17:14.52 -22:00:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 62388_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 62388_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 10724_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 10724_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 17090_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 17090_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 136162_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 136162_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:23:47.12 -15:06:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120701_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 120701_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:42:00.36 -16:20:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119291_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 119291_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 142924_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 142924_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:24:20.10 -15:27:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 09832_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 09832_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 09448_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 09448_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 197117_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 197117_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:43:29.46 -14:52:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07678_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 07678_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 135838_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 135838_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 11372_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 11372_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 108346_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 108346_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:18:32.87 -16:45:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70901_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 70901_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:39.66 -18:34:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16418_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 16418_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 162656_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 162656_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:30.57 -13:45:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75628_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 75628_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 57989_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 57989_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:16:27.52 -19:12:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142858_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 142858_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:57:09.57 -15:34:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140374_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 140374_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:37:01.40 -15:25:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25181_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 25181_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 39003_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 39003_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 12162_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 12162_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 137785_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 137785_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 63211_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 63211_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 93019_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 93019_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:45:34.21 -17:38:36.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 23025_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 23025_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 08677_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 08677_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 15294_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 15294_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 53720_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 53720_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 49659_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 49659_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:24:39.58 -19:39:40.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115936_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 115936_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 38865_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 38865_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 74429_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 74429_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 39460_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 39460_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 89550_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 89550_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 35707_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 35707_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 12811_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 12811_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:21:04.21 -22:08:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 83193_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 83193_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:51:26.25 -18:04:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.420 4120481981864491904 267.85977491133 -18.07960151982 12.7537 11.3850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 42260_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 42260_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:16:32.98 -20:03:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 17938_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 17938_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:46:25.45 -21:56:45.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 41601_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 41601_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 65527_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 65527_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:11:57.48 -18:52:14.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 46576_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 46576_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 81220_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 81220_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 15311_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 15311_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 73233_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 73233_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 85879_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 85879_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 18:04:15.13 -17:56:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 169548_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:27:45.52 -14:08:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37095_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 37095_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 122492_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 122492_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 04413_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 04413_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 47673_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 47673_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 175775_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 175775_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:21:15.16 -14:38:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 137734_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 137734_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 43788_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
Preparing report for the candidate 43788_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
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Considering the candidate 49960_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223
The candidate 49960_fd_Sgr-01-Q1b1x1_2026-04-09_03-32-53_20.00sec_-4.90C_LIGHTs_0223 did not pass the final checks
**** FOUND 17:13:31.09 -19:29:41.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 120s
Prepared the HTML report for the field Sgr-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:11:57.48 -18:52:13.9
17:58:42.50 -19:19:43.1
18:13:39.51 -19:13:06.9
17:36:54.51 -16:54:59.2
17:54:06.85 -23:03:26.6
17:51:57.93 -22:59:17.7
17:43:05.38 -22:57:20.8
17:41:51.01 -22:51:26.3
17:37:07.81 -22:48:41.6
18:00:00.21 -22:49:13.5
17:58:20.08 -22:42:53.9
17:59:20.13 -22:39:46.7
18:14:16.39 -22:33:05.0
17:38:45.30 -22:33:08.6
17:24:21.17 -22:21:47.6
17:28:13.51 -17:02:45.3
18:01:54.52 -22:28:42.3
17:24:51.05 -22:17:54.0
17:39:20.50 -16:41:05.9
17:55:47.00 -22:26:12.5
17:41:12.48 -16:39:41.5
17:54:18.44 -22:25:56.8
17:44:22.79 -16:33:24.4
17:34:12.94 -16:27:43.7
18:07:48.70 -16:24:22.8
18:13:04.77 -22:17:42.2
18:13:34.51 -16:13:50.0
17:53:37.88 -22:22:37.9
17:45:47.94 -16:07:11.0
17:25:42.03 -14:14:55.9
18:12:27.60 -15:12:04.8
18:01:11.73 -15:20:32.2
17:53:09.81 -15:19:33.1
17:57:02.98 -15:52:42.4
18:17:57.09 -22:01:12.9
17:27:43.79 -22:02:01.4
18:02:57.83 -22:01:53.6
17:35:02.01 -21:57:59.6
18:15:08.77 -21:55:13.0
18:16:49.01 -22:56:23.0
17:32:49.07 -21:41:58.8
17:50:08.78 -15:51:12.3
17:35:52.00 -16:30:22.5
18:01:12.33 -19:44:57.5
18:14:33.80 -21:51:06.0
17:40:13.58 -22:45:13.3
18:18:33.25 -23:02:27.7
18:16:49.39 -23:03:03.8
18:17:38.66 -22:46:31.4
17:22:30.23 -18:29:00.2
18:16:25.34 -18:07:10.3
18:04:53.06 -17:09:24.0
17:21:15.13 -18:24:13.0
17:27:44.78 -16:23:59.6
17:54:50.76 -21:37:10.8
18:14:19.51 -21:29:26.4
17:43:27.52 -21:25:27.6
17:29:18.68 -21:19:21.0
17:36:08.28 -21:15:56.3
18:06:12.93 -21:16:56.9
17:33:13.45 -21:11:57.2
17:48:32.73 -21:06:23.0
17:37:49.32 -20:51:51.1
17:57:09.98 -20:47:49.5
17:48:46.60 -20:45:38.1
17:21:39.43 -20:32:08.5
17:53:14.96 -20:37:59.8
17:50:06.00 -20:31:13.4
17:16:51.31 -20:16:25.2
17:29:48.17 -20:22:55.0
17:54:57.81 -20:21:00.8
17:52:17.39 -20:13:42.4
17:44:31.31 -20:11:42.0
18:03:11.49 -20:05:06.2
17:34:51.73 -19:58:35.7
17:36:50.96 -19:53:38.7
17:50:43.41 -19:49:32.0
17:13:39.30 -19:25:09.4
17:57:33.63 -19:32:22.5
17:30:49.98 -19:27:53.8
17:29:40.87 -19:22:01.9
18:09:01.25 -19:18:51.9
17:40:20.19 -19:18:03.6
17:57:02.89 -19:20:18.1
17:44:04.08 -19:13:02.2
17:24:55.32 -19:03:21.3
17:49:55.13 -19:02:12.3
17:19:51.26 -18:49:34.3
17:28:23.96 -18:54:28.5
17:36:28.38 -18:28:48.7
18:11:27.09 -18:24:54.3
18:17:29.12 -18:20:02.9
17:19:57.91 -17:59:21.6
17:50:25.65 -18:10:39.6
17:48:37.78 -18:04:55.9
17:38:01.86 -18:03:00.0
17:28:22.85 -17:41:43.1
17:45:18.41 -17:41:54.3
17:42:44.33 -17:28:54.2
########### Completed Sgr-01-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
17:58:42.50 -19:19:43.1
18:13:39.51 -19:13:06.9
17:36:54.51 -16:54:59.2
18:11:57.48 -18:52:13.9
17:50:08.78 -15:51:12.3
17:35:52.00 -16:30:22.5
18:01:12.33 -19:44:57.5
18:14:33.80 -21:51:06.0
17:40:13.58 -22:45:13.3
18:18:33.25 -23:02:27.7
18:16:49.39 -23:03:03.8
18:17:38.66 -22:46:31.4
17:22:30.23 -18:29:00.2
18:16:25.34 -18:07:10.3
18:04:53.06 -17:09:24.0
17:21:15.13 -18:24:13.0
17:27:44.78 -16:23:59.6
17:38:01.86 -18:03:00.0
17:54:50.76 -21:37:10.8
17:24:51.05 -22:17:54.0
17:19:51.26 -18:49:34.3
17:29:40.87 -19:22:01.9
17:57:09.98 -20:47:49.5
17:39:20.50 -16:41:05.9
18:02:57.83 -22:01:53.6
17:45:47.94 -16:07:11.0
17:36:08.28 -21:15:56.3
17:48:37.78 -18:04:55.9
17:41:12.48 -16:39:41.5
17:37:49.32 -20:51:51.1
17:33:13.45 -21:11:57.2
18:16:49.01 -22:56:23.0
17:50:25.65 -18:10:39.6
17:25:42.03 -14:14:55.9
17:37:07.81 -22:48:41.6
17:48:46.60 -20:45:38.1
17:48:32.73 -21:06:23.0
17:13:39.30 -19:25:09.4
17:24:55.32 -19:03:21.3
17:34:12.94 -16:27:43.7
17:57:02.98 -15:52:42.4
17:50:43.41 -19:49:32.0
17:59:20.13 -22:39:46.7
18:03:11.49 -20:05:06.2
17:32:49.07 -21:41:58.8
17:44:04.08 -19:13:02.2
17:41:51.01 -22:51:26.3
17:53:37.88 -22:22:37.9
17:51:57.93 -22:59:17.7
18:00:00.21 -22:49:13.5
17:54:06.85 -23:03:26.6
17:42:44.33 -17:28:54.2
17:52:17.39 -20:13:42.4
18:09:01.25 -19:18:51.9
18:06:12.93 -21:16:56.9
17:40:20.19 -19:18:03.6
17:54:18.44 -22:25:56.8
17:28:13.51 -17:02:45.3
17:43:27.52 -21:25:27.6
17:57:33.63 -19:32:22.5
17:35:02.01 -21:57:59.6
17:57:02.89 -19:20:18.1
17:45:18.41 -17:41:54.3
17:49:55.13 -19:02:12.3
18:01:54.52 -22:28:42.3
18:15:08.77 -21:55:13.0
18:07:48.70 -16:24:22.8
17:24:21.17 -22:21:47.6
17:38:45.30 -22:33:08.6
17:58:20.08 -22:42:53.9
18:12:27.60 -15:12:04.8
17:55:47.00 -22:26:12.5
18:17:29.12 -18:20:02.9
17:29:18.68 -21:19:21.0
17:16:51.31 -20:16:25.2
18:13:04.77 -22:17:42.2
17:53:09.81 -15:19:33.1
17:28:23.96 -18:54:28.5
18:14:19.51 -21:29:26.4
18:14:16.39 -22:33:05.0
18:17:57.09 -22:01:12.9
17:30:49.98 -19:27:53.8
17:44:22.79 -16:33:24.4
17:50:06.00 -20:31:13.4
18:11:27.09 -18:24:54.3
17:29:48.17 -20:22:55.0
17:28:22.85 -17:41:43.1
17:21:39.43 -20:32:08.5
17:54:57.81 -20:21:00.8
17:34:51.73 -19:58:35.7
17:19:57.91 -17:59:21.6
17:27:43.79 -22:02:01.4
17:36:28.38 -18:28:48.7
17:53:14.96 -20:37:59.8
18:13:34.51 -16:13:50.0
17:43:05.38 -22:57:20.8
17:36:50.96 -19:53:38.7
18:01:11.73 -15:20:32.2
17:44:31.31 -20:11:42.0
###################################################################################
17:58:42.50 -19:19:43.1 -- asteroid (will NOT add it to exclusion list)
18:13:39.51 -19:13:06.9 -- not an asteroid (will add it to exclusion list)
17:36:54.51 -16:54:59.2 -- not an asteroid (will add it to exclusion list)
18:11:57.48 -18:52:13.9 -- not an asteroid (will add it to exclusion list)
17:50:08.78 -15:51:12.3 -- not an asteroid (will add it to exclusion list)
17:35:52.00 -16:30:22.5 -- not an asteroid (will add it to exclusion list)
18:01:12.33 -19:44:57.5 -- not an asteroid (will add it to exclusion list)
18:14:33.80 -21:51:06.0 -- not an asteroid (will add it to exclusion list)
17:40:13.58 -22:45:13.3 -- not an asteroid (will add it to exclusion list)
18:18:33.25 -23:02:27.7 -- not an asteroid (will add it to exclusion list)
18:16:49.39 -23:03:03.8 -- not an asteroid (will add it to exclusion list)
18:17:38.66 -22:46:31.4 -- not an asteroid (will add it to exclusion list)
17:22:30.23 -18:29:00.2 -- asteroid (will NOT add it to exclusion list)
18:16:25.34 -18:07:10.3 -- not an asteroid (will add it to exclusion list)
18:04:53.06 -17:09:24.0 -- asteroid (will NOT add it to exclusion list)
17:21:15.13 -18:24:13.0 -- not an asteroid (will add it to exclusion list)
17:27:44.78 -16:23:59.6 -- asteroid (will NOT add it to exclusion list)
17:38:01.86 -18:03:00.0 -- not an asteroid (will add it to exclusion list)
17:54:50.76 -21:37:10.8 -- not an asteroid (will add it to exclusion list)
17:24:51.05 -22:17:54.0 -- not an asteroid (will add it to exclusion list)
17:19:51.26 -18:49:34.3 -- not an asteroid (will add it to exclusion list)
17:29:40.87 -19:22:01.9 -- asteroid (will NOT add it to exclusion list)
17:57:09.98 -20:47:49.5 -- not an asteroid (will add it to exclusion list)
17:39:20.50 -16:41:05.9 -- not an asteroid (will add it to exclusion list)
18:02:57.83 -22:01:53.6 -- not an asteroid (will add it to exclusion list)
17:45:47.94 -16:07:11.0 -- not an asteroid (will add it to exclusion list)
17:36:08.28 -21:15:56.3 -- not an asteroid (will add it to exclusion list)
17:48:37.78 -18:04:55.9 -- not an asteroid (will add it to exclusion list)
17:41:12.48 -16:39:41.5 -- not an asteroid (will add it to exclusion list)
17:37:49.32 -20:51:51.1 -- not an asteroid (will add it to exclusion list)
17:33:13.45 -21:11:57.2 -- not an asteroid (will add it to exclusion list)
18:16:49.01 -22:56:23.0 -- not an asteroid (will add it to exclusion list)
17:50:25.65 -18:10:39.6 -- not an asteroid (will add it to exclusion list)
17:25:42.03 -14:14:55.9 -- not an asteroid (will add it to exclusion list)
17:37:07.81 -22:48:41.6 -- not an asteroid (will add it to exclusion list)
17:48:46.60 -20:45:38.1 -- not an asteroid (will add it to exclusion list)
17:48:32.73 -21:06:23.0 -- not an asteroid (will add it to exclusion list)
17:13:39.30 -19:25:09.4 -- not an asteroid (will add it to exclusion list)
17:24:55.32 -19:03:21.3 -- not an asteroid (will add it to exclusion list)
17:34:12.94 -16:27:43.7 -- not an asteroid (will add it to exclusion list)
17:57:02.98 -15:52:42.4 -- not an asteroid (will add it to exclusion list)
17:50:43.41 -19:49:32.0 -- not an asteroid (will add it to exclusion list)
17:59:20.13 -22:39:46.7 -- not an asteroid (will add it to exclusion list)
18:03:11.49 -20:05:06.2 -- not an asteroid (will add it to exclusion list)
17:32:49.07 -21:41:58.8 -- not an asteroid (will add it to exclusion list)
17:44:04.08 -19:13:02.2 -- not an asteroid (will add it to exclusion list)
17:41:51.01 -22:51:26.3 -- not an asteroid (will add it to exclusion list)
17:53:37.88 -22:22:37.9 -- not an asteroid (will add it to exclusion list)
17:51:57.93 -22:59:17.7 -- not an asteroid (will add it to exclusion list)
18:00:00.21 -22:49:13.5 -- not an asteroid (will add it to exclusion list)
17:54:06.85 -23:03:26.6 -- not an asteroid (will add it to exclusion list)
17:42:44.33 -17:28:54.2 -- not an asteroid (will add it to exclusion list)
17:52:17.39 -20:13:42.4 -- not an asteroid (will add it to exclusion list)
18:09:01.25 -19:18:51.9 -- not an asteroid (will add it to exclusion list)
18:06:12.93 -21:16:56.9 -- not an asteroid (will add it to exclusion list)
17:40:20.19 -19:18:03.6 -- not an asteroid (will add it to exclusion list)
17:54:18.44 -22:25:56.8 -- not an asteroid (will add it to exclusion list)
17:28:13.51 -17:02:45.3 -- not an asteroid (will add it to exclusion list)
17:43:27.52 -21:25:27.6 -- not an asteroid (will add it to exclusion list)
17:57:33.63 -19:32:22.5 -- not an asteroid (will add it to exclusion list)
17:35:02.01 -21:57:59.6 -- not an asteroid (will add it to exclusion list)
17:57:02.89 -19:20:18.1 -- not an asteroid (will add it to exclusion list)
17:45:18.41 -17:41:54.3 -- not an asteroid (will add it to exclusion list)
17:49:55.13 -19:02:12.3 -- not an asteroid (will add it to exclusion list)
18:01:54.52 -22:28:42.3 -- not an asteroid (will add it to exclusion list)
18:15:08.77 -21:55:13.0 -- not an asteroid (will add it to exclusion list)
18:07:48.70 -16:24:22.8 -- not an asteroid (will add it to exclusion list)
17:24:21.17 -22:21:47.6 -- not an asteroid (will add it to exclusion list)
17:38:45.30 -22:33:08.6 -- not an asteroid (will add it to exclusion list)
17:58:20.08 -22:42:53.9 -- not an asteroid (will add it to exclusion list)
18:12:27.60 -15:12:04.8 -- not an asteroid (will add it to exclusion list)
17:55:47.00 -22:26:12.5 -- not an asteroid (will add it to exclusion list)
18:17:29.12 -18:20:02.9 -- not an asteroid (will add it to exclusion list)
17:29:18.68 -21:19:21.0 -- not an asteroid (will add it to exclusion list)
17:16:51.31 -20:16:25.2 -- not an asteroid (will add it to exclusion list)
18:13:04.77 -22:17:42.2 -- not an asteroid (will add it to exclusion list)
17:53:09.81 -15:19:33.1 -- not an asteroid (will add it to exclusion list)
17:28:23.96 -18:54:28.5 -- not an asteroid (will add it to exclusion list)
18:14:19.51 -21:29:26.4 -- not an asteroid (will add it to exclusion list)
18:14:16.39 -22:33:05.0 -- not an asteroid (will add it to exclusion list)
18:17:57.09 -22:01:12.9 -- not an asteroid (will add it to exclusion list)
17:30:49.98 -19:27:53.8 -- not an asteroid (will add it to exclusion list)
17:44:22.79 -16:33:24.4 -- not an asteroid (will add it to exclusion list)
17:50:06.00 -20:31:13.4 -- not an asteroid (will add it to exclusion list)
18:11:27.09 -18:24:54.3 -- not an asteroid (will add it to exclusion list)
17:29:48.17 -20:22:55.0 -- not an asteroid (will add it to exclusion list)
17:28:22.85 -17:41:43.1 -- not an asteroid (will add it to exclusion list)
17:21:39.43 -20:32:08.5 -- not an asteroid (will add it to exclusion list)
17:54:57.81 -20:21:00.8 -- not an asteroid (will add it to exclusion list)
17:34:51.73 -19:58:35.7 -- not an asteroid (will add it to exclusion list)
17:19:57.91 -17:59:21.6 -- not an asteroid (will add it to exclusion list)
17:27:43.79 -22:02:01.4 -- not an asteroid (will add it to exclusion list)
17:36:28.38 -18:28:48.7 -- not an asteroid (will add it to exclusion list)
17:53:14.96 -20:37:59.8 -- not an asteroid (will add it to exclusion list)
18:13:34.51 -16:13:50.0 -- not an asteroid (will add it to exclusion list)
17:43:05.38 -22:57:20.8 -- not an asteroid (will add it to exclusion list)
17:36:50.96 -19:53:38.7 -- not an asteroid (will add it to exclusion list)
18:01:11.73 -15:20:32.2 -- not an asteroid (will add it to exclusion list)
17:44:31.31 -20:11:42.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:13:39.30 -19:25:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:16:51.31 -20:16:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:51.26 -18:49:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:19:57.91 -17:59:21.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:15.13 -18:24:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:21:39.43 -20:32:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:24:21.17 -22:21:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:24:51.05 -22:17:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:24:55.32 -19:03:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:25:42.03 -14:14:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:27:43.79 -22:02:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:28:13.51 -17:02:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:28:22.85 -17:41:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:28:23.96 -18:54:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:29:18.68 -21:19:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:29:48.17 -20:22:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:30:49.98 -19:27:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:32:49.07 -21:41:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:33:13.45 -21:11:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:34:12.94 -16:27:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:34:51.73 -19:58:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:35:02.01 -21:57:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:35:52.00 -16:30:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:36:08.28 -21:15:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:36:28.38 -18:28:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:36:50.96 -19:53:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:36:54.51 -16:54:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:37:07.81 -22:48:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:37:49.32 -20:51:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:38:01.86 -18:03:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:38:45.30 -22:33:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:39:20.50 -16:41:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:40:13.58 -22:45:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:40:20.19 -19:18:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:41:12.48 -16:39:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:41:51.01 -22:51:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:42:44.33 -17:28:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:43:05.38 -22:57:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:43:27.52 -21:25:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:44:04.08 -19:13:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
17:44:22.79 -16:33:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:44:31.31 -20:11:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:45:18.41 -17:41:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:45:47.94 -16:07:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:48:32.73 -21:06:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:48:37.78 -18:04:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:48:46.60 -20:45:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:49:55.13 -19:02:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:06.00 -20:31:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:08.78 -15:51:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:25.65 -18:10:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:50:43.41 -19:49:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:57.93 -22:59:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:52:17.39 -20:13:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:53:09.81 -15:19:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:53:14.96 -20:37:59.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:53:37.88 -22:22:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:06.85 -23:03:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:18.44 -22:25:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:50.76 -21:37:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:57.81 -20:21:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:55:47.00 -22:26:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:02.89 -19:20:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:02.98 -15:52:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:09.98 -20:47:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:33.63 -19:32:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:58:20.08 -22:42:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:59:20.13 -22:39:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:00:00.21 -22:49:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:01:11.73 -15:20:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:01:12.33 -19:44:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:01:54.52 -22:28:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:02:57.83 -22:01:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:03:11.49 -20:05:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:12.93 -21:16:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:07:48.70 -16:24:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:01.25 -19:18:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:27.09 -18:24:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:57.48 -18:52:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:12:27.60 -15:12:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:04.77 -22:17:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:34.51 -16:13:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:13:39.51 -19:13:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:16.39 -22:33:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:19.51 -21:29:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:14:33.80 -21:51:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:15:08.77 -21:55:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:25.34 -18:07:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:49.01 -22:56:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:16:49.39 -23:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:29.12 -18:20:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:38.66 -22:46:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:17:57.09 -22:01:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:18:33.25 -23:02:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
17:13:39.30 -19:25:09.4 -- a known variable star
17:16:51.31 -20:16:25.2 -- not a known variable star
17:19:51.26 -18:49:34.3 -- a known variable star
17:19:57.91 -17:59:21.6 -- a known variable star
17:21:15.13 -18:24:13.0 -- a known variable star
17:21:39.43 -20:32:08.5 -- not a known variable star
17:24:21.17 -22:21:47.6 -- a known variable star
17:24:51.05 -22:17:54.0 -- a known variable star
17:24:55.32 -19:03:21.3 -- a known variable star
17:25:42.03 -14:14:55.9 -- a known variable star
17:27:43.79 -22:02:01.4 -- a known variable star
17:28:13.51 -17:02:45.3 -- a known variable star
17:28:22.85 -17:41:43.1 -- a known variable star
17:28:23.96 -18:54:28.5 -- a known variable star
17:29:18.68 -21:19:21.0 -- a known variable star
17:29:48.17 -20:22:55.0 -- not a known variable star
17:30:49.98 -19:27:53.8 -- a known variable star
17:32:49.07 -21:41:58.8 -- a known variable star
17:33:13.45 -21:11:57.2 -- a known variable star
17:34:12.94 -16:27:43.7 -- a known variable star
17:34:51.73 -19:58:35.7 -- a known variable star
17:35:02.01 -21:57:59.6 -- a known variable star
17:35:52.00 -16:30:22.5 -- not a known variable star
17:36:08.28 -21:15:56.3 -- a known variable star
17:36:28.38 -18:28:48.7 -- a known variable star
17:36:50.96 -19:53:38.7 -- a known variable star
17:36:54.51 -16:54:59.2 -- a known variable star
17:37:07.81 -22:48:41.6 -- a known variable star
17:37:49.32 -20:51:51.1 -- a known variable star
17:38:01.86 -18:03:00.0 -- a known variable star
17:38:45.30 -22:33:08.6 -- a known variable star
17:39:20.50 -16:41:05.9 -- a known variable star
17:40:13.58 -22:45:13.3 -- a known variable star
17:40:20.19 -19:18:03.6 -- a known variable star
17:41:12.48 -16:39:41.5 -- a known variable star
17:41:51.01 -22:51:26.3 -- a known variable star
17:42:44.33 -17:28:54.2 -- a known variable star
17:43:05.38 -22:57:20.8 -- a known variable star
17:43:27.52 -21:25:27.6 -- a known variable star
17:44:04.08 -19:13:02.2 -- a known variable star
17:44:22.79 -16:33:24.4 -- a known variable star
17:44:31.31 -20:11:42.0 -- a known variable star
17:45:18.41 -17:41:54.3 -- a known variable star
17:45:47.94 -16:07:11.0 -- a known variable star
17:48:32.73 -21:06:23.0 -- a known variable star
17:48:37.78 -18:04:55.9 -- a known variable star
17:48:46.60 -20:45:38.1 -- a known variable star
17:49:55.13 -19:02:12.3 -- not a known variable star
17:50:06.00 -20:31:13.4 -- a known variable star
17:50:08.78 -15:51:12.3 -- a known variable star
17:50:25.65 -18:10:39.6 -- a known variable star
17:50:43.41 -19:49:32.0 -- a known variable star
17:51:57.93 -22:59:17.7 -- a known variable star
17:52:17.39 -20:13:42.4 -- a known variable star
17:53:09.81 -15:19:33.1 -- a known variable star
17:53:14.96 -20:37:59.8 -- a known variable star
17:53:37.88 -22:22:37.9 -- a known variable star
17:54:06.85 -23:03:26.6 -- a known variable star
17:54:18.44 -22:25:56.8 -- a known variable star
17:54:50.76 -21:37:10.8 -- a known variable star
17:54:57.81 -20:21:00.8 -- a known variable star
17:55:47.00 -22:26:12.5 -- a known variable star
17:57:02.89 -19:20:18.1 -- a known variable star
17:57:02.98 -15:52:42.4 -- a known variable star
17:57:09.98 -20:47:49.5 -- a known variable star
17:57:33.63 -19:32:22.5 -- a known variable star
17:58:20.08 -22:42:53.9 -- a known variable star
17:59:20.13 -22:39:46.7 -- a known variable star
18:00:00.21 -22:49:13.5 -- a known variable star
18:01:11.73 -15:20:32.2 -- not a known variable star
18:01:12.33 -19:44:57.5 -- a known variable star
18:01:54.52 -22:28:42.3 -- a known variable star
18:02:57.83 -22:01:53.6 -- a known variable star
18:03:11.49 -20:05:06.2 -- a known variable star
18:06:12.93 -21:16:56.9 -- a known variable star
18:07:48.70 -16:24:22.8 -- a known variable star
18:09:01.25 -19:18:51.9 -- a known variable star
18:11:27.09 -18:24:54.3 -- a known variable star
18:11:57.48 -18:52:13.9 -- a known variable star
18:12:27.60 -15:12:04.8 -- a known variable star
18:13:04.77 -22:17:42.2 -- not a known variable star
18:13:34.51 -16:13:50.0 -- a known variable star
18:13:39.51 -19:13:06.9 -- a known variable star
18:14:16.39 -22:33:05.0 -- not a known variable star
18:14:19.51 -21:29:26.4 -- a known variable star
18:14:33.80 -21:51:06.0 -- not a known variable star
18:15:08.77 -21:55:13.0 -- a known variable star
18:16:25.34 -18:07:10.3 -- a known variable star
18:16:49.01 -22:56:23.0 -- a known variable star
18:16:49.39 -23:03:03.8 -- a known variable star
18:17:29.12 -18:20:02.9 -- a known variable star
18:17:38.66 -22:46:31.4 -- a known variable star
18:17:57.09 -22:01:12.9 -- a known variable star
18:18:33.25 -23:02:27.7 -- a known variable star
Found 9 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
94 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:13:39.30 -19:25:09.4
17:16:51.31 -20:16:25.2
17:19:51.26 -18:49:34.3
17:19:57.91 -17:59:21.6
17:21:15.13 -18:24:13.0
17:21:39.43 -20:32:08.5
17:24:21.17 -22:21:47.6
17:24:51.05 -22:17:54.0
17:24:55.32 -19:03:21.3
17:25:42.03 -14:14:55.9
17:27:43.79 -22:02:01.4
17:28:13.51 -17:02:45.3
17:28:22.85 -17:41:43.1
17:28:23.96 -18:54:28.5
17:29:18.68 -21:19:21.0
17:29:48.17 -20:22:55.0
17:30:49.98 -19:27:53.8
17:32:49.07 -21:41:58.8
17:33:13.45 -21:11:57.2
17:34:12.94 -16:27:43.7
17:34:51.73 -19:58:35.7
17:35:02.01 -21:57:59.6
17:35:52.00 -16:30:22.5
17:36:08.28 -21:15:56.3
17:36:28.38 -18:28:48.7
17:36:50.96 -19:53:38.7
17:36:54.51 -16:54:59.2
17:37:07.81 -22:48:41.6
17:37:49.32 -20:51:51.1
17:38:01.86 -18:03:00.0
17:38:45.30 -22:33:08.6
17:39:20.50 -16:41:05.9
17:40:13.58 -22:45:13.3
17:40:20.19 -19:18:03.6
17:41:12.48 -16:39:41.5
17:41:51.01 -22:51:26.3
17:42:44.33 -17:28:54.2
17:43:05.38 -22:57:20.8
17:43:27.52 -21:25:27.6
17:44:04.08 -19:13:02.2
17:44:22.79 -16:33:24.4
17:44:31.31 -20:11:42.0
17:45:18.41 -17:41:54.3
17:45:47.94 -16:07:11.0
17:48:32.73 -21:06:23.0
17:48:37.78 -18:04:55.9
17:48:46.60 -20:45:38.1
17:49:55.13 -19:02:12.3
17:50:06.00 -20:31:13.4
17:50:08.78 -15:51:12.3
17:50:25.65 -18:10:39.6
17:50:43.41 -19:49:32.0
17:51:57.93 -22:59:17.7
17:52:17.39 -20:13:42.4
17:53:09.81 -15:19:33.1
17:53:14.96 -20:37:59.8
17:53:37.88 -22:22:37.9
17:54:06.85 -23:03:26.6
17:54:18.44 -22:25:56.8
17:54:50.76 -21:37:10.8
17:54:57.81 -20:21:00.8
17:55:47.00 -22:26:12.5
17:57:02.89 -19:20:18.1
17:57:02.98 -15:52:42.4
17:57:09.98 -20:47:49.5
17:57:33.63 -19:32:22.5
17:58:20.08 -22:42:53.9
17:59:20.13 -22:39:46.7
18:00:00.21 -22:49:13.5
18:01:11.73 -15:20:32.2
18:01:12.33 -19:44:57.5
18:01:54.52 -22:28:42.3
18:02:57.83 -22:01:53.6
18:03:11.49 -20:05:06.2
18:06:12.93 -21:16:56.9
18:07:48.70 -16:24:22.8
18:09:01.25 -19:18:51.9
18:11:27.09 -18:24:54.3
18:11:57.48 -18:52:13.9
18:12:27.60 -15:12:04.8
18:13:04.77 -22:17:42.2
18:13:34.51 -16:13:50.0
18:13:39.51 -19:13:06.9
18:14:16.39 -22:33:05.0
18:14:19.51 -21:29:26.4
18:14:33.80 -21:51:06.0
18:15:08.77 -21:55:13.0
18:16:25.34 -18:07:10.3
18:16:49.01 -22:56:23.0
18:16:49.39 -23:03:03.8
18:17:29.12 -18:20:02.9
18:17:38.66 -22:46:31.4
18:17:57.09 -22:01:12.9
18:18:33.25 -23:02:27.7
17:50:37.96 -17:56:28.0
17:43:00.78 -16:46:37.7
17:47:19.03 -17:30:47.6
17:31:15.36 -21:35:45.4
17:41:30.07 -20:41:22.4
17:27:29.25 -14:49:34.5
18:00:34.73 -22:59:32.0
17:49:36.33 -16:55:58.5
17:44:52.39 -16:33:31.1
18:17:57.06 -20:40:01.0
17:23:12.69 -18:59:04.4
17:29:00.13 -17:45:13.7
17:41:31.13 -17:03:17.3
17:29:28.95 -19:16:36.3
17:41:29.39 -16:25:51.6
18:14:59.87 -23:11:06.8
17:41:01.59 -15:28:53.8
17:18:52.22 -22:00:26.6
17:52:32.65 -23:08:15.5
17:43:06.10 -22:56:54.2
17:45:29.50 -16:46:38.8
17:49:43.72 -15:52:01.5
17:46:25.45 -21:56:45.4
17:17:24.05 -13:07:04.5
17:42:01.45 -18:32:47.2
18:11:27.07 -22:32:28.0
17:16:03.93 -15:26:01.5
18:15:49.69 -22:08:23.0
18:18:17.53 -22:47:57.2
18:18:26.45 -22:09:48.4
18:17:13.39 -21:59:07.2
18:17:32.52 -22:07:44.1
18:18:15.06 -22:02:23.5
17:52:55.97 -22:53:35.3
17:34:16.75 -22:21:19.2
17:36:00.23 -21:04:59.9
17:46:04.13 -22:29:00.5
17:47:36.02 -19:36:48.2
17:17:30.04 -16:15:14.5
17:46:29.81 -16:15:26.2
17:23:26.16 -17:44:59.1
17:20:10.77 -20:28:26.9
17:37:10.34 -16:36:53.1
17:39:19.67 -20:09:05.1
17:35:56.41 -18:55:47.8
17:41:32.91 -16:20:44.9
17:46:43.31 -22:58:40.7
17:16:17.35 -14:58:52.0
18:14:10.97 -17:22:14.9
18:07:14.04 -21:03:56.5
18:14:28.25 -16:24:43.6
17:16:38.26 -12:35:00.3
17:39:16.62 -13:37:39.1
17:48:46.63 -16:11:19.3
18:01:06.83 -21:00:05.7
17:44:37.45 -15:23:12.4
17:17:46.41 -13:03:51.9
17:20:32.87 -12:46:42.4
18:03:12.49 -20:18:37.5
18:04:40.99 -15:13:24.7
17:16:02.64 -19:18:41.7
18:14:01.89 -20:23:33.3
17:59:41.02 -21:00:29.9
18:12:43.68 -15:52:05.1
17:52:20.87 -21:37:38.9
18:17:05.62 -18:40:06.5
18:17:15.85 -20:16:03.9
18:14:08.73 -15:10:59.1
18:17:27.23 -18:49:47.8
18:18:24.73 -17:59:40.3
17:12:57.45 -21:47:20.7
18:10:34.22 -15:42:12.6
18:15:16.06 -22:25:56.8
18:18:20.51 -22:06:43.0
18:16:19.50 -21:37:54.2
18:17:06.53 -20:19:03.6
18:18:18.40 -21:53:46.7
18:18:42.10 -16:31:20.6
17:15:37.49 -20:02:59.3
18:14:24.14 -23:10:44.9
18:06:19.54 -16:41:17.8
18:18:28.11 -22:56:04.3
18:18:29.04 -22:52:41.3
18:17:36.94 -22:56:01.1
18:14:59.89 -23:11:06.8
18:18:29.58 -23:06:33.8
18:16:39.94 -23:10:04.2
18:17:24.60 -22:53:51.7
18:18:35.89 -22:34:58.0
18:18:35.43 -21:53:08.8
18:18:38.60 -13:45:55.4
18:08:24.03 -23:14:24.3
18:17:26.32 -23:07:50.5
18:18:31.53 -22:21:24.3
18:18:18.75 -22:50:45.6
18:18:24.36 -22:19:33.9
18:17:11.57 -22:46:04.4
18:18:01.23 -23:05:16.4
18:18:07.34 -23:05:29.6
17:59:26.00 -15:09:14.3
18:18:03.63 -22:57:35.9
17:15:38.02 -17:12:20.6
18:18:06.03 -22:32:42.0
17:41:53.76 -16:26:35.7
18:01:12.78 -15:19:58.0
18:17:05.55 -23:03:04.8
18:17:55.10 -18:19:32.4
18:12:25.82 -15:25:09.8
17:40:29.71 -20:01:26.1
17:21:38.35 -14:37:31.8
18:04:53.49 -16:01:16.8
17:35:52.24 -18:34:24.3
17:51:06.92 -13:09:34.8
17:23:40.22 -22:36:02.5
18:14:45.03 -21:19:48.8
17:44:40.61 -15:16:19.1
17:40:50.54 -16:21:01.7
18:03:55.89 -15:23:28.7
17:51:38.45 -20:50:39.2
18:04:28.52 -18:57:41.1
18:01:15.38 -16:13:02.8
17:52:06.87 -21:48:51.0
17:40:28.82 -13:34:31.7
17:35:01.62 -19:13:32.3
17:39:55.60 -21:55:25.3
17:38:39.24 -15:24:51.3
18:04:16.40 -17:20:42.9
17:44:18.74 -23:04:08.2
17:45:34.93 -15:03:31.3
17:44:05.64 -13:29:07.2
17:20:03.00 -18:32:09.2
17:50:56.46 -22:15:36.0
17:49:21.55 -17:06:27.0
17:56:22.68 -19:10:39.8
17:25:45.59 -15:48:16.9
17:33:13.57 -18:50:49.1
17:25:31.05 -18:00:59.8
18:03:07.45 -15:19:57.6
17:48:09.86 -20:37:30.1
17:44:11.94 -19:23:22.6
18:11:09.22 -18:55:16.7
17:22:53.20 -20:18:09.9
17:38:59.50 -22:30:53.3
17:30:50.24 -22:44:10.4
17:28:25.25 -21:02:38.1
17:38:14.09 -15:21:50.1
17:49:30.53 -21:51:17.8
17:43:21.55 -15:18:22.6
17:51:06.33 -18:38:44.5
17:49:32.35 -15:28:50.4
17:26:33.66 -20:28:42.6
17:42:14.31 -13:26:38.3
17:39:05.77 -20:34:28.6
17:33:47.95 -16:15:48.8
17:42:35.20 -17:04:48.2
17:55:08.20 -23:07:10.2
17:42:27.06 -21:41:26.6
17:39:50.62 -18:40:16.4
17:29:24.35 -16:24:42.9
17:34:14.60 -19:17:00.3
17:58:13.48 -20:02:53.7
18:00:02.81 -14:48:42.1
17:38:00.57 -20:29:47.4
17:35:29.80 -16:01:40.9
17:38:28.99 -14:31:03.6
17:36:42.30 -17:16:38.0
17:30:47.99 -18:27:18.8
17:25:49.50 -16:21:16.9
18:18:51.32 -19:32:31.0
18:18:24.40 -18:39:27.0
17:51:26.25 -18:04:49.7
17:38:16.82 -17:55:37.3
17:45:34.21 -17:38:36.9
17:46:10.04 -15:45:28.6
18:17:51.56 -21:49:42.3
18:15:50.00 -23:10:18.4
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The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461139.85545819 -observatory V36
23:34:22.15 -05:15:37.5 Mercury (0.2mag)
02:36:31.81 +15:12:37.9 Venus (-3.9mag)
23:58:56.32 -01:13:02.8 Mars (1.2mag)
07:09:51.02 +22:50:40.4 Jupiter (-2.1mag)
00:26:11.82 +00:30:16.8 Saturn (0.9mag)
03:46:20.29 +19:43:05.6 Uranus (5.8mag)
00:09:57.49 -00:20:57.0 Neptune (7.8mag)
20:33:25.39 -22:52:26.9 Pluto (14.5mag)
18:47:03.28 -28:03:03.5 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Apr 9 03:34 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461139.85545819:
07:09:58.73 +22:50:25.6 Io (5.7mag)
07:10:02.13 +22:50:18.9 Europa (5.9mag)
07:10:03.39 +22:50:09.4 Ganymede (5.3mag)
07:09:21.84 +22:51:43.0 Callisto (6.5mag)
07:13:27.43 +22:41:32.1 Himalia (15.3mag)
07:09:49.58 +22:50:41.0 Thebe (16.2mag)
07:13:29.73 +23:10:55.7 Elara (17.3mag)
07:08:16.77 +23:34:09.3 Pasiphae (17.4mag)
07:18:19.17 +22:47:59.3 Carme (18.5mag)
00:26:19.19 +00:30:06.0 Titan (8.8mag)
00:26:15.67 +00:30:27.7 Rhea (10.1mag)
00:26:05.19 +00:31:26.6 Iapetus (11.5mag)
00:26:23.65 +00:30:03.4 Hyperion (14.8mag)
00:27:53.80 +00:39:46.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 03:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.85545819:
15:04:48.30 -11:09:02.2 JWST
17:51:55.15 +37:17:21.1 Chandra
18:50:02.20 -18:48:49.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 03:35 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.85545819 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:53.80 -28:24:14.2 13.9mag P/2010 H2 (Vales)
05:02:08.20 -69:59:10.0 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:07.03 +31:23:40.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.21 +09:45:11.2 17.6mag C/2021 G2 (ATLAS)
23:08:20.35 +28:58:39.1 17.0mag C/2022 E2 (ATLAS)
04:21:34.46 +25:51:15.5 15.9mag C/2022 N2 (PANSTARRS)
09:02:14.20 +31:57:18.0 16.2mag C/2022 QE78 (ATLAS)
08:30:14.25 -00:52:30.1 17.3mag C/2022 R6 (PANSTARRS)
18:55:05.97 +17:58:04.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:40.69 -11:37:01.9 17.6mag P/2023 B1 (PANSTARRS)
09:11:00.12 -12:58:10.9 17.6mag C/2023 F3 (ATLAS)
21:47:08.95 +62:32:04.2 17.5mag C/2023 H5 (Lemmon)
19:24:22.31 -03:38:25.9 14.2mag C/2023 R1 (PANSTARRS)
21:41:11.72 +85:00:53.1 17.8mag C/2023 X2 (Lemmon)
06:15:19.57 +63:33:16.2 17.1mag C/2024 A1 (ATLAS)
04:58:31.48 +15:53:15.1 10.6mag C/2024 E1 (Wierzchos)
16:23:20.31 +05:17:54.2 17.4mag C/2024 G6 (ATLAS)
20:18:43.18 +13:30:06.8 14.7mag C/2024 J3 (ATLAS)
03:20:29.49 -23:24:59.7 16.4mag C/2024 T5 (ATLAS)
05:11:12.51 +46:59:15.0 17.7mag C/2025 J1 (Borisov)
14:06:21.28 +40:23:59.7 14.9mag C/2025 L1 (ATLAS)
03:15:02.32 -25:12:19.4 17.8mag C/2025 Q3 (ATLAS)
23:03:29.52 +19:45:47.1 9.6mag C/2025 R3 (PANSTARRS)
12:57:00.68 +02:35:51.3 17.5mag C/2025 Y1 (ATLAS)
02:19:41.43 +03:41:19.7 10.4mag C/2026 A1 (MAPS)
23:40:18.98 +35:55:22.1 14.4mag C/2026 B2 (Sun-Gao)
18:29:58.61 -10:03:53.8 12.2mag 10P/Tempel
15:09:02.48 +03:50:54.1 13.4mag 24P/Schaumasse
11:04:44.00 -01:45:00.8 15.7mag 29P/Schwassmann-Wachmann
17:58:26.18 -09:51:55.4 17.8mag 40P/Vaisala
10:38:14.36 -04:39:30.5 16.8mag 43P/Wolf-Harrington
01:38:24.93 +16:20:46.9 17.2mag 47P/Ashbrook-Jackson
06:58:47.10 +38:25:20.3 17.0mag 63P/Wild
23:20:28.73 -12:15:38.4 15.7mag 65P/Gunn
03:45:46.51 +18:54:22.2 15.9mag 76P/West-Kohoutek-Ikemura
00:50:58.11 +06:54:55.5 14.4mag 78P/Gehrels
22:42:33.29 -11:20:58.2 14.6mag 88P/Howell
01:51:49.72 +18:50:04.8 15.1mag 93P/Lovas
04:42:32.61 +31:55:00.0 16.3mag 123P/West-Hartley
08:21:00.63 +41:25:44.1 16.2mag 124P/Mrkos
02:23:00.98 +13:37:13.1 16.4mag 128P/Shoemaker-Holt
02:34:32.81 +13:39:48.8 17.5mag 131P/Mueller
00:51:47.06 +10:49:49.1 11.0mag 141P/Machholz
01:01:30.21 +02:22:41.4 11.0mag 141P-A/Machholz
23:50:15.04 -01:25:10.8 13.6mag 141P-D/Machholz
01:31:06.23 +04:05:21.2 17.9mag 141P-I/Machholz
00:43:54.12 -04:51:07.0 15.2mag 162P/SidingSpring
10:30:03.07 +31:18:27.5 17.9mag 164P/Christensen
06:24:13.91 +24:26:38.3 17.9mag 198P/ODAS
15:03:12.26 -00:48:24.3 17.4mag 210P/Christensen
21:18:56.58 -13:03:24.6 17.5mag 218P/LINEAR
17:14:14.06 -14:42:58.7 16.2mag 235P/LINEAR
05:20:17.07 +34:09:04.9 16.6mag 240P/NEAT
07:35:27.35 -05:54:43.8 17.7mag 242P/Spahr
15:45:00.31 +06:32:10.9 17.5mag 391P/Kowalski
07:31:51.36 +21:20:05.4 17.6mag 450P/LONEOS
05:26:19.71 +45:25:22.5 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 03:35 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
-rw-r--r-- 1 apache apache 5.8K Apr 9 03:34 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 03:34 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
15:50:43.720 +47:30:42.19 AT 2026ify 2026-03-30.81 21.34
17:38:02.570 +25:54:11.91 AT 2026ifx 2026-03-27.88 20.89
16:42:02.490 +40:59:30.50 AT 2026ifw 2026-03-27.86 21.32
16:24:14.050 +39:37:35.59 AT 2026ifv 2026-03-27.86 20.81
16:16:45.660 +38:01:36.33 AT 2026ifu 2026-03-27.86 21.15
16:28:23.190 +36:11:26.67 AT 2026ift 2026-03-27.86 21.53
16:16:10.610 +36:40:26.87 AT 2026ifs 2026-03-27.86 20.03
16:42:08.700 +33:28:34.26 AT 2026ifr 2026-03-27.86 21.24
16:45:41.760 +34:10:06.31 AT 2026ifq 2026-03-27.86 21.64
16:50:17.550 +33:04:52.33 AT 2026ifp 2026-03-27.86 19.99
16:52:21.140 +31:25:32.03 AT 2026ifo 2026-03-27.86 19.73
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
16:26:20.250 +28:06:35.30 AT 2026ifm 2026-03-27.85 20.13
17:01:36.800 +29:43:13.81 AT 2026ifl 2026-03-27.85 20.62
17:06:26.770 +28:47:25.16 AT 2026ifk 2026-03-27.85 21.39
16:47:18.680 +27:13:25.92 AT 2026ifj 2026-03-27.85 20.26
15:55:49.720 +37:36:32.33 AT 2026ifi 2026-03-24.80 21.32
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
-rw-r--r-- 1 apache apache 30K Apr 9 03:34 tns_transients_list.txt
